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Jodrell B survey

Jodrell B survey


The Jodrell B survey (jb2) published its results in papers published from 1981 to 1992 with a total of 41 new pulsars discovered. It detected a grand total of 20 pulsars. The fastest pulsar discovered was J1833-0827 with a period of 85.28815 milliseconds and the slowest pulsar was J1852+0031 with a period of 2.1802 seconds. The smallest pulsar dispersion measure was J1738-3211 with a DM of 49.59 pc/cc and the largest pulsar dispersion measure was J1852+0031 with a DM of 787.0 pc/cc. There were a total of 324 pulsars known before the first discovery was published. This survey increased the total amount of known pulsars by 13.0%.

There were 59 papers written about the discoveries of this survey: High-Sensitivity Pulsar Survey, Discovery of a pulsar in a binary system, Deep sample of new pulsars and their spatial extent in the Galaxy, millisecond pulsar, New millisecond pulsar in a binary system, Results of Two Surveys for Fast Pulsars, Millisecond pulsar in an eclipsing binary, Two Newly Discovered Millisecond Pulsars, Search for Fast Pulsars along the Galactic Plane, PSR 1257+12 and PSR 1534+12, nearby 37.9-ms radio pulsar in a relativistic binary system, Discovery of Two Fast-rotating Pulsars, Two Newly Discovered Millisecond Pulsars, Search for Pulsars at High Galactic Latitudes, Search for Millisecond Pulsars., High Galactic Latitude Pulsar Survey of the Arecibo Sky, Search for extrasolar planetary systems., Search for Millisecond Pulsars at Galactic Latitudes -50 degrees < B < -20 degrees, Princeton-Arecibo Declination-Strip Survey for Millisecond Pulsars. I., Survey for Millisecond Pulsars, Discovery of Three Radio Pulsars from an X-Ray--selected Sample, The Green Bank Northern Sky Survey for Fast Pulsars, Searching for FAST Pulsars, PSR J1829+2456: a relativistic binary pulsar, Arecibo Timing and Single-Pulse Observations of Eighteen Pulsars, Arecibo timing and single-pulse observations of 17 pulsars, Discovery of 10 pulsars in an Arecibo drift-scan survey, PSR J1453+1902 and the radio luminosities of solitary versus binary millisecond pulsars, No pulsar left behind - I. Timing, pulse-sequence polarimetry and emission morphology for 12 pulsars, Arecibo Pulsar Survey Using ALFA. I. Survey Strategy and First Discoveries, Arecibo Pulsar Survey Using ALFA. II. The Young, Highly Relativistic Binary Pulsar J1906+0746, An Eccentric Binary Millisecond Pulsar in the Galactic Plane, PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV γ-Ray Source HESS J1857+026, Arecibo Pulsar Survey Using ALFA: Probing Radio Pulsar Intermittency And Transients, Pulsar Discovery by Global Volunteer Computing, Arecibo PALFA Survey and Einstein@Home: Binary Pulsar Discovery by Volunteer Computing, Two Millisecond Pulsars Discovered by the PALFA Survey and a Shapiro Delay Measurement, Four Highly Dispersed Millisecond Pulsars Discovered in the Arecibo PALFA Galactic Plane Survey, Timing and Interstellar Scattering of 35 Distant Pulsars Discovered in the PALFA Survey, Timing of Five Millisecond Pulsars Discovered in the PALFA Survey, Einstein@Home Discovery of a PALFA Millisecond Pulsar in an Eccentric Binary Orbit, Arecibo Pulsar Survey Using ALFA. IV. Mock Spectrometer Data Analysis, Survey Sensitivity, and the Discovery of 40 Pulsars, PALFA Single-pulse Pipeline: New Pulsars, Rotating Radio Transients, and a Candidate Fast Radio Burst, Eight Millisecond Pulsars Discovered in the Arecibo PALFA Survey, Goals, Strategies and First Discoveries of AO327, the Arecibo All-sky 327 MHz Drift Pulsar Survey, New Discoveries from the Arecibo 327 MHz Drift Pulsar Survey Radio Transient Search, Pulsar J1411+2551: A Low-mass Double Neutron Star System, The Discovery of Six Recycled Pulsars from the Arecibo 327 MHz Drift-Scan Pulsar Survey, Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT, Eight γ-ray Pulsars Discovered in Blind Frequency Searches of Fermi LAT Data, Precise γ-ray Timing and Radio Observations of 17 Fermi γ-ray Pulsars, PSR J0007+7303 in the CTA1 Supernova Remnant: New Gamma-Ray Results from Two Years of Fermi Large Area Telescope Observations, iscovery of Nine Gamma-Ray Pulsars in Fermi Large Area Telescope Data Using a New Blind Search Method, PSR J1838-0537: Discovery of a Young, Energetic Gamma-Ray Pulsar, Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations, Einstein@Home Discovery of Four Young Gamma-Ray Pulsars in Fermi LAT Data, Three Millisecond Pulsars in Fermi LAT Unassociated Bright Sources, Discovery of millisecond pulsars in radio searches of southern Fermi Large Area Telescope sources, 350-MHz GBT Survey of 50 Faint Fermi γ-ray Sources for Radio Millisecond Pulsars.


PSRs discovered by the Jodrell B survey

JNAMESPIN PERIODDMMAGNETIC FIELD STRENGTH
J1738-3211 768.499 milliseconds 49.59 pc/cc 7.91e+11 G
J1739-2903 322.886 milliseconds 138.55 pc/cc 1.61e+12 G
J1739-3131 529.441 milliseconds 596.9 pc/cc 3.17e+12 G
J1740-3015 606.887 milliseconds 151.96 pc/cc 1.7e+13 G
J1753-2501 528.336 milliseconds 672.0 pc/cc 2.76e+12 G
J1756-2435 670.48 milliseconds 367.1 pc/cc 4.42e+11 G
J1803-2137 133.667 milliseconds 233.99 pc/cc 4.29e+12 G
J1808-2057 918.41 milliseconds 606.8 pc/cc 4.01e+12 G
J1809-2109 702.414 milliseconds 381.91 pc/cc 1.66e+12 G
J1812-1718 1.205 seconds 251.4 pc/cc 4.85e+12 G
J1812-1733 538.341 milliseconds 509.8 pc/cc 7.36e+11 G
J1816-1729 782.313 milliseconds 520.7 pc/cc 2.41e+12 G
J1818-1422 291.489 milliseconds 619.65 pc/cc 7.8e+11 G
J1820-1346 921.46 milliseconds 771.0 pc/cc 2.06e+12 G
J1822-1400 214.771 milliseconds 649.27 pc/cc 4.47e+11 G
J1824-1118 435.759 milliseconds 601.31 pc/cc 1.26e+12 G
J1825-1446 279.198 milliseconds 352.23 pc/cc 2.55e+12 G
J1826-1131 2.093 seconds 320.58 pc/cc 3.24e+12 G
J1826-1334 101.487 milliseconds 231.0 pc/cc 2.8e+12 G
J1827-0958 245.757 milliseconds 430.0 pc/cc 5.02e+11 G
J1830-1059 405.073 milliseconds 159.7 pc/cc 4.99e+12 G
J1832-0827 647.326 milliseconds 300.87 pc/cc 6.51e+12 G
J1832-1021 330.354 milliseconds 474.14 pc/cc 1.19e+12 G
J1833-0827 85.288 milliseconds 410.95 pc/cc 8.95e+11 G
J1835-0643 305.83 milliseconds 464.8 pc/cc 3.56e+12 G
J1836-0436 354.237 milliseconds 231.5 pc/cc 7.76e+11 G
J1837-0653 1.906 seconds 316.1 pc/cc 1.23e+12 G
J1841-0425 186.149 milliseconds 325.49 pc/cc 1.1e+12 G
J1842-0359 1.84 seconds 195.98 pc/cc 9.78e+11 G
J1844-0244 507.722 milliseconds 422.13 pc/cc 2.95e+12 G
J1844-0433 991.027 milliseconds 123.16 pc/cc 1.99e+12 G
J1844-0538 255.704 milliseconds 411.71 pc/cc 1.59e+12 G
J1845-0434 486.751 milliseconds 230.8 pc/cc 2.38e+12 G
J1852+0031 2.18 seconds 787.0 pc/cc 1.47e+13 G
J1857+0212 415.823 milliseconds 506.77 pc/cc 4.14e+12 G
J1901+0716 643.999 milliseconds 252.81 pc/cc 1.23e+12 G
J1902+0615 673.505 milliseconds 502.9 pc/cc 2.31e+12 G
J1905+0709 648.04 milliseconds 245.34 pc/cc 1.81e+12 G
J1906+0641 267.275 milliseconds 472.8 pc/cc 7.65e+11 G
J2002+3217 696.761 milliseconds 142.21 pc/cc 8.66e+12 G

Binary PSRs discovered by the Jodrell B survey

JNAMESPIN PERIODDMMAGNETIC FIELD STRENGTHORBITAL PERIODECCENTRICITY
J1823-1115 279.829 milliseconds 428.59 pc/cc 6.29e+11 G 357.762 days 0.795

PSRs detected by the Jodrell B survey

JNAMESPIN PERIODDMMAGNETIC FIELD STRENGTH
J1745-3040 367.434 milliseconds 88.37 pc/cc 2e+12 G
J1752-2806 562.558 milliseconds 50.37 pc/cc 2.16e+12 G
J1757-2421 234.106 milliseconds 179.45 pc/cc 1.77e+12 G
J1759-2205 460.982 milliseconds 177.16 pc/cc 2.26e+12 G
J1847-0402 597.809 milliseconds 141.98 pc/cc 5.63e+12 G
J1848-0123 659.432 milliseconds 159.1 pc/cc 1.88e+12 G
J1901+0331 655.45 milliseconds 402.08 pc/cc 2.24e+12 G
J1902+0556 746.577 milliseconds 177.49 pc/cc 3.14e+12 G
J1909+1102 283.642 milliseconds 149.98 pc/cc 8.76e+11 G
J1915+1009 404.552 milliseconds 241.69 pc/cc 2.51e+12 G
J1916+0951 270.254 milliseconds 60.95 pc/cc 8.35e+11 G
J1916+1312 281.845 milliseconds 237.01 pc/cc 1.03e+12 G
J1917+1353 194.631 milliseconds 94.54 pc/cc 1.2e+12 G
J1918+1444 1.181 seconds 27.2 pc/cc 1.6e+13 G
J1921+1419 618.183 milliseconds 91.64 pc/cc 1.88e+12 G
J1926+1434 1.325 seconds 211.41 pc/cc 5.46e+11 G
J1926+1648 579.823 milliseconds 176.88 pc/cc 3.27e+12 G
J1932+2020 268.217 milliseconds 211.15 pc/cc 1.08e+12 G
J1954+2923 426.677 milliseconds 7.93 pc/cc 2.73e+10 G
J2004+3137 2.111 seconds 234.82 pc/cc 1.27e+13 G